This work presents the structural
decomposition of a sample of 11 disk galaxies, which span a range of different
morphological types.
The U, B, V, R, and I photometric
information given in Paper I
(color and color-index images and luminosity,
ellipticity, and position-angle profiles) has been used to decide
what types of components form the galaxies
before carrying out the decomposition. We find and model such components as
bulges, disks, bars, lenses and rings.

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